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1. | Binding energy per nucleon is practically constant for nuclei with mass numbers between \(30\) and \(170\). |
2. | Binding energy per nucleon is maximum for \(_{56}\mathrm{Fe}\) (equal to \(8.75~\text{MeV}\)). |
3. | Binding energy per nucleon for \(_{6}\mathrm{Li}\) is lower compared to \(_{4}\mathrm{He}\). |
4. | Higher the binding energy per nucleon, the more unstable is the nucleus. |
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Assertion (A): | The density of the nucleus is much higher than that of ordinary matter. |
Reason (R): | \(10^5\) times smaller. | Most of the mass of the atom is concentrated in the nucleus while the size of this nucleus is almost
1. | Both (A) and (R) are True and (R) is the correct explanation of (A). |
2. | Both (A) and (R) are True but (R) is not the correct explanation of (A). |
3. | (A) is True but (R) is False. |
4. | Both (A) and (R) are False. |
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1. | kinetic energy | 2. | mass |
3. | momentum | 4. | all the above |
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1. | \(E_1\): total binding energy of initial nuclei |
2. | \(E_2\): total binding energy of final nuclei |
3. | \(A_1\): total number of nucleons of initial nuclei |
4. | \(A_2\): total number of nucleons of final nuclei |
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1. | \(_2\mathrm{He}^4\) | 2. | \(_3\mathrm{Li}^8\) |
3. | \(_4\mathrm{Be}^8\) | 4. | \(_8\mathrm{O}^{16}\) |
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1. | the outermost atomic shell |
2. | the innermost atomic shell |
3. | the conduction band |
4. | the nucleus |
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1. | some nucleons are created |
2. | some nucleons are destroyed |
3. | energy is converted into mass |
4. | mass is converted into energy |
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1. | \(r_{_X}=r_{_Y}+r_{_Z}\) | 2. | \(\Large\frac{1}{r_{_X}}=\frac{1}{r_{_Y}}+\frac{1}{r_{_Z}}\) |
3. | \(r_{_X}=|r_{_Y}-r_{_Z}|\) | 4. | \(r_{_X}^3=r^3_{_Y}+r^3_{_Z}\) |
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